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Astron. Astrophys. 336, 654-661 (1998)

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Acknowledgements

The work of FK was supported by APART (Austrian Programme for Advanced Research and Technology) from the Austrian Academy of Sciences. FK was also supported by the Fonds zur Förderung der wissenschaftlichen Forschung under project number S7308-AST and the Österreichische Nationalbank under the Jubiläumsfonds-project number 6876. HO acknowledges financial support from the Swedish Natural Science Research Council.

The authors are very grateful to Göran Sandell for carefully performing the JCMT observations, and thank Martin Groenewegen for providing us with the IRAM spectra of CZ Ser. The reduction of the CO spectra was made using the DRP software kindly provided by Michael Olberg, OSO.

The Swedish-ESO Submillimetre Telescope, SEST, is operated jointly by ESO and the Swedish National Facility for Radio Astronomy, Onsala Space Observatory at Chalmers University of Technology. The James Clerk Maxwell Telescope is operated by The Joint Astronomy Centre on behalf of the Particle Physics and Astronomy Research Council of the United Kingdom, the Netherlands Organisation for Scientific Research, and the National Research Council of Canada. This research has made use of the SIMBAD database.

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© European Southern Observatory (ESO) 1998

Online publication: July 20, 1998
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